Composition of the Secondary Particles Produced in Nuclear Interactions at ∼1012eV

1964 ◽  
Vol 136 (2B) ◽  
pp. B515-B528 ◽  
Author(s):  
C. O. Kim
1968 ◽  
Vol 46 (5) ◽  
pp. 343-358 ◽  
Author(s):  
B. Judek

Interaction mean free paths of relativistic secondary particles emitted from interactions of heavy primary cosmic-ray nuclei in emulsions were measured. The results show that among the Be, Li, He, and singly charged secondary nuclei there are particles present which interact with a cross section several times higher than the expected geometrical value. The stars produced by these particles have the characteristics of ordinary nuclear interactions. There appears to be no interpretation of these observations in terms of any known particle phenomena.


1968 ◽  
Vol 46 (10) ◽  
pp. S1128-S1129
Author(s):  
A. M. Abdullaev ◽  
S. A. Azimov ◽  
H. Zaynutdinov ◽  
E. Mulladzhanov ◽  
T. S. Yuldashbaev

A description is given of the installation which was constructed at an altitude of 3 200 m for the study of nuclear interactions at energies of 1012–1013 eV. The apparatus, which has an effective area of 10 m2, includes an ionization calorimeter and a Cerenkov total absorption spectrometer for the measurement of the energies of the primary particles, a μ-meson detector consisting of Cerenkov counters and spark chambers, and also a spark chamber for the study of the angular distribution of secondary particles.


1964 ◽  
Vol 32 (4) ◽  
pp. 873-879 ◽  
Author(s):  
P. L. Jain ◽  
H. C. Glahe ◽  
J. D. Rinaldo ◽  
P. D. Bharadwaj

1963 ◽  
Vol 28 (6) ◽  
pp. 1238-1245 ◽  
Author(s):  
E. Farrow ◽  
C. F. Gauld ◽  
C. B. A. McCusker ◽  
J. Malos ◽  
K. Nishikawa ◽  
...  

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